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  • 1
    Monograph available for loan
    Monograph available for loan
    Cambridge : Cambridge University Press
    Call number: PIK N 322-99-0127
    Type of Medium: Monograph available for loan
    Pages: 336 p.
    Edition: 1. ed.
    ISBN: 0521598370
    Branch Library: PIK Library
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  • 2
    Electronic Resource
    Electronic Resource
    [s.l.] : Nature Publishing Group
    Nature 412 (2001), S. 237-244 
    ISSN: 1476-4687
    Source: Nature Archives 1869 - 2009
    Topics: Biology , Chemistry and Pharmacology , Medicine , Natural Sciences in General , Physics
    Notes: [Auszug] There is substantial evidence that the martian volatile inventory and climate have changed markedly throughout the planet's history. Clues come from areas as disparate as the history and properties of the deep interior, the composition of the crust and regolith, the morphology of the surface, ...
    Type of Medium: Electronic Resource
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  • 3
    Electronic Resource
    Electronic Resource
    [s.l.] : Nature Publishing Group
    Nature 370 (1994), S. 328-329 
    ISSN: 1476-4687
    Source: Nature Archives 1869 - 2009
    Topics: Biology , Chemistry and Pharmacology , Medicine , Natural Sciences in General , Physics
    Notes: [Auszug] THE martian surface has geological features that suggest that the climate has changed substantially during its history. High erosion rates and the presence of valley networks on the older geological units - some seen in the photograph below - are usually interpreted as signs that abundant liquid ...
    Type of Medium: Electronic Resource
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  • 4
    Electronic Resource
    Electronic Resource
    [s.l.] : Nature Publishing Group
    Nature 315 (1985), S. 559-561 
    ISSN: 1476-4687
    Source: Nature Archives 1869 - 2009
    Topics: Biology , Chemistry and Pharmacology , Medicine , Natural Sciences in General , Physics
    Notes: [Auszug] That some mechanism must exist for replenishment of the equatorial inventory of water has been suspected on several grounds: (1) if the valleys formed in a manner analogous to terrestrial river valleys, by slow erosion of running water, then the volumes of water that would have flowed through them ...
    Type of Medium: Electronic Resource
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  • 5
    facet.materialart.
    Unknown
    In:  Other Sources
    Publication Date: 2019-01-25
    Description: The behavior of water vapor in the atmosphere of Mars is important to understanding the Mars climate and its evolution as well as the nature of ongoing seasonal processes of exchange and transport. On the seasonal timescales, exchange of water between the atmosphere, regolith, and polar caps combine with advection of water and the possible saturation at some locations and seasons in order to produce the observed distribution of water. A summary of the observations made by the Mariner and Viking spacecraft and analyses of the seasonal cycle of water is presented, along with a brief discussion of the implications for the long term variability of water. The upcoming Mars Observer mission is also briefly discussed.
    Keywords: LUNAR AND PLANETARY EXPLORATION
    Type: Lunar and Planetary Inst., MECA Workshop on Atmospheric H2O Observations of Earth and Mars. Physical Processes, Measurements and Interpretations; p 53
    Format: text
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  • 6
    Publication Date: 2019-01-25
    Description: It is noted that while the SME (Solar Mesosphere Explorer) data is consistent with the earlier LIMS (Limb Infrared Monitor of the Stratosphere) results, its interpretation is complicated by aerosol contamination, particularly at altitudes below 35 km. This contamination arose from several volcanic eruptions, including that of El Chichon. Analyses are reported of a subset of data from the SME satellite, concentrating primarily on the period January through March 1982 so as to avoid contamination from the El Chichon volcanic aerosol. The SME observations of water vapor between 20 and 60 km were inverted for the first three months of 1982 as well as for selected additional periods. Reasonable results are obtained at locations where no contamination by aerosol is suspected.
    Keywords: GEOPHYSICS
    Type: Lunar and Planetary Inst., MECA Workshop on Atmospheric H2O Observations of Earth and Mars. Physical Processes, Measurements and Interpretations; p 54-55
    Format: text
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  • 7
    Electronic Resource
    Electronic Resource
    [s.l.] : Nature Publishing Group
    Nature 415 (2002), S. 733-734 
    ISSN: 1476-4687
    Source: Nature Archives 1869 - 2009
    Topics: Biology , Chemistry and Pharmacology , Medicine , Natural Sciences in General , Physics
    Notes: [Auszug] ...Astrobiology burst upon the world in the mid-1990s, as the excitement about possible life on Mars recorded in the meteorite ALH84001 (ref. 1) and the discovery of planetary systems around other stars received intense international attention. Was the answer to the question that has been ...
    Type of Medium: Electronic Resource
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  • 8
    facet.materialart.
    Unknown
    In:  CASI
    Publication Date: 2013-08-31
    Description: The long-term evolution of both the atmosphere and the surface of Mars can be understood by examining the history of volatiles in the Mars atmosphere, their non-atmospheric reservoirs, and the processes of exchange between the two. Clearly, the present state of both the surface and the atmosphere can only be seen, so that any inferences about the evolution of the climate system are just that, inferences. The processes which control the atmosphere and surface on a seasonal basis, however, are the same processes which can act on longer timescales; only the specific solar and atmospheric forcing will differ. Once the ability of each process to affect the seasonal behavior is understood, the long-timescale forcing may be applied to the various processes in order to clearly identify the ability of the processes to act over the entire history of Mars. The areas of surface-atmospheric interaction of Mars are addressed in the ongoing research. The climate system on Mars is controlled by processes involving the exchange between the surface and atmosphere, so it is important to understand the current behavior of those processes. This is especially so in light of the current interest in understanding Mars; the upcoming Mars Observer mission, and the potential for a future sample-return or human-exploration mission will focus emphasis on this area of Mars science.
    Keywords: LUNAR AND PLANETARY EXPLORATION
    Type: NAS 1.26:183113 , NASA-CR-183113
    Format: application/pdf
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  • 9
    facet.materialart.
    Unknown
    In:  CASI
    Publication Date: 2013-08-31
    Description: The recent focus in Mars research was in the area of the seasonal behavior of water in the atmosphere, surface, and polar caps, and exchange of water between these reservoirs. Results of recent work is summarized.
    Keywords: LUNAR AND PLANETARY EXPLORATION
    Type: NASA-CR-180249 , NAS 1.26:180249
    Format: application/pdf
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  • 10
    Publication Date: 2013-08-31
    Description: Researchers investigated the physical properties of the Martian surface as inferred from a combination of orbiting and earth-based remote sensing observations and in-situ observations. This approach provides the most detailed and self-consistent view of the global and regional nature of the surface. Results focus on the areas of modeling the diurnal variation of the surface temperature of Mars, incorporating the effects of atmospheric radiation, with implications for the interpretation of surface thermal inertia; modeling the thermal emission from particulate surfaces, with application to observations of the surfaces of the Earth, Moon, and Mars; modeling the reflectance spectrum of Mars in an effort to understand the role of particle size in the difference between the bright and dark regions; and determining the slope properties of different terrestrial surfaces and comparing them with planetary slopes derived from radar observations.
    Keywords: LUNAR AND PLANETARY EXPLORATION
    Type: NASA, Washington, Reports of Planetary Geology and Geophysics Program, 1990; p 229-230
    Format: application/pdf
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